Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-18T10:33:27.382Z Has data issue: false hasContentIssue false
  • English
  • Français

9.9. Extended UV emission in NGC6251

Published online by Cambridge University Press:  25 May 2016

Philippe Crane  and
Joel Vernet
Philippe Crane
Affiliation:
European Southern Observatory Garching, Germany
Joel Vernet
Affiliation:
European Southern Observatory Garching, Germany

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

NGC 6251 is an optically normal elliptical galaxy that hosts one of the most spectacular radio jets(Perley, Bridle, and Willis, 1984). This jet extends about 1 Mpc and its axis is roughly perpendicular to the central dust ring. NGC6251 was originally observed with HST in a survey of elliptical galaxies(Crane et al., 1993) and revealed an anamoly which was pursued in the investigation reported here.

Type
Part III. Black Holes and Central Activity
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 399 - 400
Copyright
Copyright © Kluwer 1998 

References

Blackman, E. and Yi, I.,(1996) Ap.J. 461 L21.CrossRefGoogle Scholar
Crane, P., et al.,(1993) AJ. 106, 1371.Google Scholar
Crane, P., and Vernet, J.,(1997) Ap.J. 496,L91.CrossRefGoogle Scholar
Perley, R.A., Bridle, A.H., and Willis, A.G., (1984) Ap.JS., 54,291.Google Scholar